Evolution of M81 with Exponentially Decreasing Star Formation Rate of PEGASE

Based on the large field multicolor observations of Beijing-Arizona-Taiwan-Connecticut (BATC) program, we obtain the spectral energy distribution (SED) for individual regions of M81. We study the structure and evolution of M81 with an evolutionary population synthesis (EPS) model, PEGASE. We find that the exponentially deceasing star formation rate (SFR) with star formation scale 3 Gyr (hereafter Exp, τ=3 Gyr) gives the best agreement between the model predictions and the observed SEDs. We then obtain the structure, age distribution and evolutionary history of M81. There is a clear age gradient between the central and outer regions. The populations in the central regions are older than 7 Gyr,those in the outer regions are younger, at about 4.5 Gyr. The youngest components in the spiral arms have ages of about 2.5 Gyr or less.     

国家基础测绘成果情况介绍

介绍了现存于国家基础地理信息中心的国家基础测绘成果情况，为广大测绘工作者了解和在工作中利用提供方便。     

Age and Mass Estimates for 41 Star Clusters in M33

In this second paper of our series, we estimate the age of 41 star clusters, which were detected by Melnick & D'odorico in the nearby spiral galaxy M33, by comparing the integrated photometric measurements with theoretical stellar population synthesis models of Bruzual & Chariot. Also, we calculate the mass of these star clusters using the theoretical M/Lv ratio. The results show that, these star clusters formed continuously in M33 from ~ 7×106 - 1010 years and have masses between ~ 103 and 2×106 M⊙. M33 frames were observed as a part of the BATC Multicolor Survey of the sky in 13 intermediate-band niters from 3800 to 10 OOOA. The relation between age and mass confirms that the sample star cluster masses systematically decrease from the oldest to the youngest.     

Advanced analyses of 57Fe Mössbauer data of alumino-silicate glasses

⁵⁷Fe Mössbauer spectra of iron bearing alumino-silicate glasses are analysed by two complementary methods (SID and x-VBF) especially adapted for the analysis of disordered systems by taking into account distributions of hyperfine Mössbauer parameters. Qualitative and quantitative information about the oxidation state of iron are obtained as well as information about the distribution of local environments of iron. The possibility to separate the signal of ferric iron from that of ferrous iron allows to derive precise redox ratio in favourable cases but also to analyse more sharply the different contributions to Mössbauer spectra. Using two different glass series (feldspar composition, haplo-tonalitic composition), the characteristics of the two methods are described and employed to study the effect of composition, water incorporation and oxidation state on the glass structure. Optical absorption spectroscopy is used to support the interpretation of the Mössbauer spectra in case of the feldspar glasses.     

无线传感器网络监测中远程数据传输的GPRS实现

无线传感器网络在大面积监控如煤田火灾、煤田水位遥测中有着广阔的应用前景,其中将数据从监控点传输到监控中心是一个关键环节。为了解决远程数据传输问题,在无线传感器汇聚节点上添加了GPRS模块。传感器采集的信号传到汇聚节点,由单片机ATmega128控制,通过GPRS模块SIM100发送到GPRS网,最终送到与Internet相连的计算机终端。介绍了单片机的串口通信以及发送数据的过程,给出了部分程序,并对系统进行了测试。结果表明,该系统能够实现实时的数据传输。     

岩石弹性模量对钻孔体应变仪M2波视潮汐因子影响分析

首先,应用 Venedikow 调和分析方法计算体应变仪观测记录的M2波视潮汐因子;然后,对体应变仪井下传感器观测层岩芯进行单轴压缩试验,根据应力-应变曲线求取岩芯试样的力学参数。对比研究试样的单轴抗压强度和弹性模量与M2波视潮汐因子的关系,结果表明,弹性模量E对M2波视潮汐因子有明显的影响,随着M2波视潮汐因子的增大,岩石弹性模量呈线性函数降低,二者具有很好的相关性。钻孔岩芯力学性质的差异性是造成体应变仪之间M2波视潮汐因子差异较大的主要因素。